• 천문학회보
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• 제45권1호
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• pp.36.2-36.2
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• 2020

Intensive Monitoring Survey of Nearby Galaxies (IMSNG) has been managed over 6 years. It aimed to constrain the progenitor system and explosion mechanism of SNe by detection of very early signal from shock heated emission. We have conducted monitoring observation of nearby bright galaxies those were carefully selected using global network of 1-m class telescopes. More than 20 SNe have occured in our target fields. As One of result of the survey, we present light curve analysis of type Ia SN 2018kp, which was discovered in NGC 3367. Based on photometric analysis, we calculated explosion parameters and set constraints of physical conditions of this supernova. We compared the results with theoretical model progenitor systems to find out which scenario is the most fitted to SN 2018kp case. Moreover, we estimate the distance to the galaxy and look into the relation between SNe and galactic physical parameters.

• 한국정보과학회논문지:소프트웨어및응용
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• 제37권9호
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• pp.669-675
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• 2010

이른 시스템 개발 단계에서 요구사항 에러를 찾기 위해서는 시스템의 행위가 정형 언어로 표현되어야 하고, 도달성 분석이나 싸이클 탐색과 같은 분석 기술로 분석해야 한다. 하지만 이 기술들은 시스템의 상태 공간 순회를 기반으로 하기 때문에 시스템이 복잡해지면 상태 폭발 문제가 발생할 수 있다. 즉, 순회를 위한 메모리와 수행 시간이 큰 상태 공간 때문에 기하 급수적으로 증가한다. 본 논문에서는 병행 시스템에서 이러한 문제가 나타나는 원인을 지적하고 순회에 필요한 메모리를 줄이기 위해서 병행적 상태 공간을 합성하지 않고 순회한다. 또한 수행 시간을 줄이기 위해서 방문 기록을 최소한으로 유지하는 새로운 기술을 제시한다. 마지막으로 이 기법이 효과적임을 실험 결과를 통해 보인다.

• 한국항공우주학회지
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• 제44권8호
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• pp.741-757
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• 2016

구 소련이 달에 루나(Luna) 1호를 발사한 이래 달을 비롯한 지구 밖의 천체에 대한 우주탐사를 시작한 지 60년이 된 지금 인류는 아직 외계의 생명체는 발견하지 못하였으나 태양계의 거의 모든 행성을 근접거리에서 탐사하고 빠른 속도로 이동하는 혜성의 표면에 우주선을 착륙시키는 등 괄목할 만한 성과를 이룩하였다. 그렇지만 아직까지 사람이 외계에 착륙한 곳은 달 뿐이며, 미국을 비롯한 여러 나라들이 사람을 달 또는 화성에 보내 기지를 건설하고 생존할 수 있도록 하는 것을 목표로 우주탐사에 매진하고 있다. 한편, 1990년대 초반에 우주개발을 시작한 우리나라는 정부주도로 수립된 수차례의 우주개발계획에서 달 탐사를 포함한 우주탐사계획을 선언하고 달 탐사 계획을 박근혜정부의 국정과제로 추진하여 2016년 초 공식적으로 달 탐사 프로그램을 시작하였다. 본 논문에서는 우리나라 달 탐사계획과 세계 우주탐사 프로그램의 간략한 역사, 관련기술의 발전현황과 개발방향 등을 살펴본다. 아울러 우리나라의 우주탐사분야의 과학연구 현황 및 분야별 기술수준을 점검한다.

• Archives of Reconstructive Microsurgery
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• 제17권1호
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• pp.19-27
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• 2008

Purpose: Microvascular reconstructive surgery has become an integral part of the treatment of head and neck cancer patients. This review of 121 free flaps for head and neck cancer patients performed over the last 11 years was done to evaluate circulatory crisis, salvage, and secondary reconstruction and to investigate which factors may contribute to these rates. Method: Nine emergent explorations among 121 head and neck reconstruction with free flaps were reviewed to analyze detection of vascular crisis, the time interval from detection of circulatory crisis to exploration, operation procedures and results, and secondary reconstructions. Emergent exploration was done with our protocol. Result: Nine free flaps exhibited signs of vascular problems between 1 day and 6 days postoperatively. The emergent exploration rate of this series was 7.4% (9/121). The salvage rate was 55.6% (5/9), giving an overall flap viability of 96.7% (117/121). In our study, preoperative radiation therapy, positive smoking history, alcohol consumption history, combined disease such as diabetes mellitus and hypertension, recipient vessels and types of vascular anastomosis were not related to the causes of circulatory crisis. The mean time interval between the onset of clinical recognition of impaired flap perfusion and re-exploration of the salvaged 5 flaps was 3.2 hours, that of failed 4 flaps was 11.25 hours. Conclusion: Despite high overall success rate, relatively low salvage rate may be attributed to late detection of circulatory crisis and in long time interval between detection and exploration. We conclude that early detection of circulatory crisis and expeditious re-exploration are a matter of great importance for the success of salvage operation.

• 천문학회보
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• 제44권2호
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• pp.76.1-76.1
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• 2019

After the first identification of electromagnetic counterpart of gravitational wave source (GW170817), era of multi-messenger astronomy has begun. For specifying coordinate, magnitude, and host galaxy information, optical follow-up observation of GW source becomes important. The O3 run of LIGO / VIRGO started after April 2019. We present searching strategy of GW optical counterpart using the KMTNet. By performing tiling observation of high probability area in GW localization map, we expect to observe early light-curve of GW optical counterpart. We will also present observation result for three gravitational wave events of binary black hole mergers. After identification of optical counterpart, we will study collision mechanism, progenitor, and characteristics of host galaxy using observation data of GW source.

• 천문학회보
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• 제42권1호
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• pp.34.3-35
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• 2017

Spectral energy distribution camera for QUasars in EArly uNiverse (SQUEAN) is a successor of Camera for Quasars in EArly uNiverse (CQUEAN) which was developed by Center for the Exploration of the Origin of the Universe and operated at the 2.1 m Otto Struve Telescope in the McDonald Observatory, USA, since 2010. The software of SQUEAN controls a science camera, a guiding camera, and a filter wheel, and communicates with the telescope control system (TCS). It has been constantly revised and modularized according to the upgrades of the TCS and the hardware changes. Recently we have implemented the stable network communication and the semi-automatic focusing modules to enhance observational convenience. In this presentation we describe the current status of the SQUEAN control software and introduce a software architecture which is optimized on efficient astronomical observations.

• 자원환경지질
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• 제55권2호
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• pp.149-169
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• 2022

인도네시아 석탄은 중국, 인도, 한국 등 아시아의 주요 국가들에서 에너지원으로써 널리 소비되고 있다. 민간기업들의 높은 수요로 인해, 인도네시아 석탄 탐사사업은 해외자원개발 조사사업을 통해 가장 많이 지원된 국가이자 광종이다. 본 논문에서는 석탄 탐사를 통해 그동안 축적된 탐사자료를 활용하여 인도네시아 함탄분지와 함탄층의 특성에 대해 종합하여 고찰하고자 한다. 인도네시아의 동부 깔리만탄과 수마트라의 신생대 제3기 퇴적분지들은 동아시아에서 가장 생산적인 함탄분지들이다. 주요 탄층의 산출특성은 지질시대별로 차이를 보인다. 깔리만탄의 바리또 분지와 아셈아셈 분지 내 에오세 탄층들은 탄폭은 얇고 부존 매수가 적은 경향이 있으나, 고열량의 양호한 탄질로 인하여 일찍부터 주요 탐사대상이었다. 후기 올리고세-전기 마이오세 탄층들은 소규모로 부존하지만, 중소규모의 탄광으로 개발하기에 적합하다. 동부 깔리만탄과 수마트라에 걸쳐 광역적으로 분포하는 마이오세-플라이오세 탄층들은 낮은 열량에도 불구하고, 두꺼운 탄폭과 다량의 부존매수의 이점을 활용하여 활발히 개발되고 있다. 다양한 사례들은 효율적이고 성공적인 탐사를 위해 함탄층의 지질학적 부존여건에 대한 전반적인 이해가 선행될 필요가 있음을 보여준다. 본 논문에서 제공하는 인도네시아 함탄분지와 함탄층에 대한 전문학술정보는 향후 우리나라 기업들의 탐사활동에 유용한 참고자료로 활용될 것으로 기대된다.

• 천문학논총
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• 제27권4호
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• pp.287-288
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• 2012

Radio-loud active galaxies have been found to exhibit a close connection to galactic mergers and host galaxy star-formation quenching. We present preliminary results of an optical spectroscopic investigation of the AKARI NEP field. We focus on the population of radio-loud AGN and use photometric and spectroscopic information to study both their star-formation and nuclear activity components. Preliminary results show that radio-AGN are associated with early type, massive galaxies with relatively old stellar populations.

• International Journal of Aeronautical and Space Sciences
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• 제16권4호
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• pp.624-635
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• 2015

Design space exploration has been much neglected in aircraft conceptual design phase, which often leads to a waste of time and cost in design, manufacture and operation process. It is necessary to explore design space based on operational system-of-systems (SoS) simulation during the early phase for a competitive design. This paper proposes a methodology to analyze aircraft performance parameters in four steps: combination of parameters, object analysis, operational simulation, and key-parameters analysis. Meanwhile, the design space of an unmanned aerial vehicle applied in earthquake search and rescue SoS is explored based on this methodology. The results show that applying SoS simulation into design phase has important reference value for designers on aircraft conceptual design.

• 천문학회보
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• 제41권1호
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• pp.71.1-71.1
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• 2016

Photometric reverberation mapping is an effective alternative to time consuming spectroscopy. It usually employs narrow bands to track the luminosity variations of broad emission lines, such as Balmer lines, and broadbands for the continuum variability. Here, we investigate the feasibility of substituting these for medium bands, with 50nm widths, that are currently being used on the SED Camera for QUasars in EArly uNiverse (SQUEAN) installed on the 2.1m Otto Struve Telescope at McDonald Observatory. Three targets with recent variability and/or short expected time lags were selected, and observed for 15 minutes each in the medium band containing $H{\alpha}$, and the two adjacent bands for continuum subtraction afterwards. Analysis shows that for one of the objects, SDSS J0350+0037, the pure $H{\alpha}$ emission line flux has a S/N ~ 12, so that variabilities up to ~ 8% are detectable. Thus, future observations using these medium bands on SQUEAN seem to be practical.